NGC 4788 is a globular cluster located in the constellation Centaurus. It is approximately 50,000 light-years away from Earth and is estimated to be around 12 billion years old. This cluster contains a large number of stars, with its core being densely packed, making it a fascinating object for astronomers. Discovered by James Dunlop in 1826, NGC 4788 is notable for its unique characteristics, including a high concentration of metal-poor stars. Its appearance is somewhat irregular compared to other globular clusters, which adds to its intrigue in the study of stellar evolution and the formation of galaxies.